atnu8 said:
This book is great! I love how it's written. I just read chapter 4: Trip to Canopus and found that extremely enlightening, thank you for sharing.
I appreciate all of you for being patient with me!
How does this sound:
All measurements of time are dilated when moving at high speed relative to an inertial observer.
(Time slows down for moving observers compared to non-moving observers)
You seem to be stuck on the idea that "time slows down". One can ask "Slows down relative to what? To me, your words suggest you believe in some sort of "absolute time" in which things can be at "absolute rest", this viewpoint has been presented by you several times and hasn't changed through the thread in spite of our efforts to explain that it's not the viewpoint of special relativity. But I'll repeat for emphasis that this is not the viewpoint of special relativity. This, my take on what you are saying is that when you talk about "time slowing down", you think that the time you measure with your clock slows down relative to some sort of absolute time. While such absolute time is present in Newtonian theory, it is NOT present in special relativity. Therfore, if you want to understand special relativity, you need to abandon this notion of absolute time. This make take some effort.
I'll try and break down the concept of time in special relativity. There are at least two sorts of time in special relativity. One is proper time. THis is the sort of time measured with a clock. A clock can be regarded as "travelling through spacetime", and, a bit like a wristwatch, if the clock is present and two events at different times, it will give a reading as to the time difference between the two events.
The second notion of time is different from the above. It's the notion of "simultaneous events". When a clock is not physically present at both events, one needs such a notion to measure the time interval between said events.
There is possibly a third notion related to time here, the notion of causality. But I won't be going into that in this post.
Separating and disambiguiting the two notions of time (proper time and simultaneity) are I think the most that it is reasonable to address in one post.
I will describe my view of "time dilation", and, if you are capable of drawing space-time diagrams, I'd encourage you to draw them. If you're not capable, I'd encourage learning how to draw them. You'll need the related concepts of "events" and "worldlines".
To do this, you will need both of the concepts I outlined - the notion of "proper time" and the notion of "simuttaneity" or "now". And I'll be using some concepts which are standard in space-time diagram, namely events (which happen at some specific time and place), and worldlines (which are the set of all events that some observer experiences).
Draw two worldlines on a space-time diagram, A and B. We'll regard one worldline, worldine A, as our reference. You might call it "stationary". And the second worldine B is a worldine of "an observer moving relative to A". If you're familir with the distinction, we are talking about "timelike worldlines" here, worldlines that are a one-dimensional set of events that an observer "experiences".
Along worldine A, using a clock, we mark regular proper time intervals. Because it's a proper time interval, it has a length, which we measure with a clock. We'll call this interval t_a.
For every point on worldline A, we find the unique event on worldline B that occurs "at the same time" as the event on worldline A. To do this, we need a notion of simutaneity, of events that occur "at the same time", a concept of now. There's a formal way we do this in specail relativty, we use what we call Einstein's clock synchronization convention, and to apply this convention proeprly, we need to specify a specific frame or observer in which we will apply this convention.
These events that we mark along worldline B turn out to also occur at regular intervals of proper time on worldine B, but the value of this interval (which we again measure with a clock) is t_b, which is in general different from t_a. The ratio of t_b to t_a is then the time dilation.
Einstein clock synchronization is important here, and if you haven't studied it, it's something you need to study to grasp special realtivity. The easiest way to study is is to draw space-time diagrams. To provide some physical insight for the space-time diagrams, you need to know how to measure time intervals (proper time intervals0 on the diagram, how to measure space intervals on the diagram (distances with a ruler), and how to synchronize clocks (the Einstein clock syncrhonization method). You need to be able to do all th ree.
We are perfectly free to exhcange the roles of A and B. When we do so, though, it turns out t he process of Einstein clock syncrhonization depends on our choice. The correspondence of points on worldline A to worldine B is a map. The map between A to B in A's frame is different from the map between A and B in B's frame, so when we interchange the observers, we use a dfferent map. THis is important.
Your second point involves GR and not SR. The short answer is that you got this one right, but discussing it at length would make thyis post too long - it's already probalby presenting too much material.